MID-INFRARED GALAXY MORPHOLOGY FROM THE <i>SPITZER</i> SURVEY OF STELLAR STRUCTURE IN GALAXIES (S <sup>4</sup> G): THE IMPRINT OF THE DE VAUCOULEURS REVISED HUBBLE-SANDAGE CLASSIFICATION SYSTEM AT 3.6 μm
R. Buta(University of Alabama), Taehyun Kim(Seoul National University), J. H. Knapen(University of Hertfordshire), H. Salo(University of Oulu), S. Comerón(University of Oulu), A. Gil de Paz(Universidad Complutense de Madrid), A. Bosma(Centre National de la Recherche Scientifique), J. L. Hinz, D. M. Elmegreen(Vassar College), Luis C. Ho(Peking University), Dimitri A. Gadotti, E. Athanassoula(Laboratoire d’Astrophysique de Marseille), Karín Menéndez‐Delmestre(Universidade Federal do Rio de Janeiro), Kartik Sheth(National Radio Astronomy Observatory), Karen L. Masters(University of Portsmouth), Manuel Aravena, Michael W. Regan(Space Telescope Science Institute), Barry F. Madore(Carnegie Observatories), Mark Seibert(Carnegie Observatories), J. C. Muñoz-Mateos(University of Arizona), E. Laurikainen(University of Turku)
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